Output files:
Pass | File name | Description | Start date, UT range | Antennas | Polarizations | # subbands (AIPS IFs) | Bandwidth per IF (MHz) | Spectral channels per IF/pol | Corr. int. time (s) |
---|---|---|---|---|---|---|---|---|---|
v558c-vla1 | V558C.VLA1.FITS | Continuum. All sources. VLA-MID at position of VLA1 | 2019-02-28, 0/04:30:00 - 0/14:59:59 | AT CD HH HO KM MP PA T6 WA | RR LL RL LR | 8 | 16.0 MHz | 64 | 1.0 |
v558c-vla2 | V558C.VLA2.FITS | Continuum. VLA-MID at position of VLA2 | 2019-02-28, 0/06:00:20 - 0/14:57:40 | AT CD HH HO KM MP PA T6 WA | RR LL RL LR | 8 | 16.0 MHz | 64 | 1.0 |
v558c-gated | V558C.GATED.FITS | Gated pass. VLA-MID at position of J0437 | 2019-02-28, 0/06:00:20 - 0/14:57:40 | AT CD HH HO KM MP PA T6 WA | RR LL RL LR | 8 | 16.0 MHz | 64 | 1.0 |
CD: no fringes after 2019y05905h20m. Probably a recorder problem.
KM: no fringes after 2019y059d08h09m40s. Reason unknown, but suspected to be a pointing issue.
Correlator: Data from 2019y059d04h30m00s until 2019y059d05h50m00s are included to help diagnose a possible pointing problem at KM. However, as this is nominally telescope setup time, these scans should not be used for general calibration (e.g. manual delay cal) as the telescope configurations may be unstable during this period.
Correlator: The pulsar is gated on phase 0.83 to 0.85 in the gated pass. The pipeline shows that the pulsar is well detected indicating the ephemeris and gate are good.
Plots of autocorrelations
Comments:
Plots of uncalibrated amplitude and phase against frequency
Comments:
Plots of uncalibrated amplitude and phase against time
Comments:
Plots of cross-polarization amplitude and phase against frequency (not always available)
Comments:
Amplitude corrections from ACCOR
Comments:
Fringe-fit delay solutions
Comments:
Fringe-fit phase solutions
Comments:
Fringe-fit rate solutions
Comments:
Fringe-fit SNR
Comments:
Plots of Amplitude and phase against frequency with fringe-fit solutions applied
Comments:
Plots of Amplitude and phase against time with fringe-fit solutions applied
Comments:
Plots of autocorrelations
Comments:
Plots of uncalibrated amplitude and phase against frequency
Comments:
Plots of uncalibrated amplitude and phase against time
Comments:
Plots of cross-polarization amplitude and phase against frequency (not always available)
Comments:
Amplitude corrections from ACCOR
Comments:
Fringe-fit delay solutions
Comments:
Fringe-fit phase solutions
Comments:
Fringe-fit rate solutions
Comments:
Fringe-fit SNR
Comments:
Plots of Amplitude and phase against frequency with fringe-fit solutions applied
Comments:
Plots of Amplitude and phase against time with fringe-fit solutions applied
Comments:
Plots of autocorrelations
Comments:
Plots of uncalibrated amplitude and phase against frequency
Comments:
Plots of uncalibrated amplitude and phase against time
Comments:
Plots of cross-polarization amplitude and phase against frequency (not always available)
Comments:
Amplitude corrections from ACCOR
Comments:
Fringe-fit delay solutions
Comments:
Fringe-fit phase solutions
Comments:
Fringe-fit rate solutions
Comments:
Fringe-fit SNR
Comments:
Plots of Amplitude and phase against frequency with fringe-fit solutions applied
Comments:
Plots of Amplitude and phase against time with fringe-fit solutions applied
Comments: